Search results for "TRANSFORMATION"

showing 10 items of 1634 documents

Cosmological Perturbations in Renormalization Group Derived Cosmologies

2002

A linear cosmological perturbation theory of an almost homogeneous and isotropic perfect fluid Universe with dynamically evolving Newton constant $G$ and cosmological constant $\Lambda$ is presented. A gauge-invariant formalism is developed by means of the covariant approach, and the acoustic propagation equations governing the evolution of the comoving fractional spatial gradients of the matter density, $G$, and $\Lambda$ are thus obtained. Explicit solutions are discussed in cosmologies where both $G$ and $\Lambda$ vary according to renormalization group equations in the vicinity of a fixed point.

PhysicsHigh Energy Physics - TheoryIsotropyAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsPerfect fluidCosmological constantAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsFixed pointRenormalization groupAstrophysicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Space and Planetary ScienceHomogeneousCosmological perturbation theoryCovariant transformationMathematical PhysicsMathematical physics
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Observable traces of non-metricity: new constraints on metric-affine gravity

2018

Relaxing the Riemannian condition to incorporate geometric quantities such as torsion and non-metricity may allow to explore new physics associated with defects in a hypothetical space-time microstructure. Here we show that non-metricity produces observable effects in quantum fields in the form of 4-fermion contact interactions, thereby allowing us to constrain the scale of non-metricity to be greater than 1 TeV by using results on Bhabha scattering. Our analysis is carried out in the framework of a wide class of theories of gravity in the metric-affine approach. The bound obtained represents an improvement of several orders of magnitude to previous experimental constraints.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsScatteringPhysics beyond the Standard ModelFOS: Physical sciencesTorsion (mechanics)ObservableGeneral Relativity and Quantum Cosmology (gr-qc)16. Peace & justice01 natural scienceslcsh:QC1-999General Relativity and Quantum CosmologyGravitationTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesNuclear and High Energy Physics; theories of gravity; geometric quantitiesAffine transformation010306 general physicsQuantumlcsh:Physics
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Running Newton Constant, Improved Gravitational Actions, and Galaxy Rotation Curves

2004

A renormalization group (RG) improvement of the Einstein-Hilbert action is performed which promotes Newton's constant and the cosmological constant to scalar functions on spacetime. They arise from solutions of an exact RG equation by means of a ``cutoff identification'' which associates RG scales to the points of spacetime. The resulting modified Einstein equations for spherically symmetric, static spacetimes are derived and analyzed in detail. The modifications of the Newtonian limit due to the RG evolution are obtained for the general case. As an application, the viability of a scenario is investigated where strong quantum effects in the infrared cause Newton's constant to grow at large …

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics (astro-ph)Dark matterFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantNewtonian limitAstrophysicsGeneral Relativity and Quantum CosmologyGravitationsymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Einstein field equationssymbolsSchwarzschild metricWeyl transformationGalaxy rotation curveMathematical physics
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Quantum cosmological approach to 2d dilaton gravity

1993

We study the canonical quantization of the induced 2d-gravity and the pure gravity CGHS-model on a closed spatial section. The Wheeler-DeWitt equations are solved in (spatially homogeneous) choices of the internal time variable and the space of solutions is properly truncated to provide the physical Hilbert space. We establish the quantum equivalence of both models and relate the results with the covariant phase-space quantization. We also discuss the relation between the quantum wavefunctions and the classical space-time solutions and propose the wave function representing the ground state.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsCanonical quantizationHilbert spaceFOS: Physical sciencesSpace (mathematics)Quantization (physics)symbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)symbolsDilatonCovariant transformationWave functionQuantumGeneral Theoretical PhysicsMathematical physics
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Modular transformations of elliptic Feynman integrals

2021

We investigate the behaviour of elliptic Feynman integrals under modular transformations. This has a practical motivation: Through a suitable modular transformation we can achieve that the nome squared is a small quantity, leading to fast numerical evaluations. Contrary to the case of multiple polylogarithms, where it is sufficient to consider just variable transformations for the numerical evaluations of multiple polylogarithms, it is more natural in the elliptic case to consider a combination of a variable transformation (i.e. a modular transformation) together with a redefinition of the master integrals. Thus we combine a coordinate transformation on the base manifold with a basis transf…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsClass (set theory)Basis (linear algebra)010308 nuclear & particles physicsbusiness.industryCoordinate systemFOS: Physical sciencesModular designBase (topology)01 natural sciencesManifoldAlgebraHigh Energy Physics - PhenomenologyTransformation (function)High Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)0103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsbusinessVariable (mathematics)
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Yang-Mills two-point functions in linear covariant gauges

2015

In this work we use two different but complementary approaches in order to study the ghost propagator of a pure SU(3) Yang-Mills theory quantized in the linear covariant gauges, focusing on its dependence on the gauge-fixing parameter $\xi$ in the deep infrared. In particular, we first solve the Schwinger-Dyson equation that governs the dynamics of the ghost propagator, using a set of simplifying approximations, and under the crucial assumption that the gluon propagators for $\xi>0$ are infrared finite, as is the case in the Landau gauge $(\xi=0)$. Then we appeal to the Nielsen identities, and express the derivative of the ghost propagator with respect to $\xi$ in terms of certain auxiliary…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics - Lattice (hep-lat)PropagatorFOS: Physical sciencesFísicaYang–Mills existence and mass gapRotation formalisms in three dimensionsGluonHigh Energy Physics - PhenomenologyHigh Energy Physics::TheoryHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanicsCovariant transformationMathematical physicsGauge fixingAnsatz
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Entropy function from toric geometry

2021

It has recently been claimed that a Cardy-like limit of the superconformal index of 4d $\mathcal{N}=4$ SYM accounts for the entropy function, whose Legendre transform corresponds to the entropy of the holographic dual AdS$_5$ rotating black hole. Here we study this Cardy-like limit for $\mathcal{N}=1$ toric quiver gauge theories, observing that the corresponding entropy function can be interpreted in terms of the toric data. Furthermore, for some families of models, we compute the Legendre transform of the entropy function, comparing with similar results recently discussed in the literature.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciQuiverFOS: Physical sciencesToric varietyBlack hole entropy Black hole microstates superconformal index AdS/CFTQC770-798Binary entropy functionLegendre transformationEntropy (classical thermodynamics)symbols.namesakeHigh Energy Physics - Theory (hep-th)Rotating black holeNuclear and particle physics. Atomic energy. RadioactivitysymbolsLimit (mathematics)Gauge theoryMathematical physicsNuclear Physics B
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Ghosts in metric-affine higher order curvature gravity

2019

We disprove the widespread belief that higher order curvature theories of gravity in the metric-affine formalism are generally ghost-free. This is clarified by considering a sub-class of theories constructed only with the Ricci tensor and showing that the non-projectively invariant sector propagates ghost-like degrees of freedom. We also explain how these pathologies can be avoided either by imposing a projective symmetry or additional constraints in the gravity sector. Our results put forward that higher order curvature gravity theories generally remain pathological in the metric-affine (and hybrid) formalisms and highlight the key importance of the projective symmetry and/or additional co…

PhysicsHigh Energy Physics - TheoryPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsFOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)Curvature01 natural sciencesRotation formalisms in three dimensionsGeneral Relativity and Quantum CosmologyFormalism (philosophy of mathematics)Theoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical scienceslcsh:QB460-466lcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityAffine transformationProjective test010306 general physicsEngineering (miscellaneous)Ricci curvatureEuropean Physical Journal C: Particles and Fields
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Scattering amplitudes in affine gravity

2020

Affine gravity is a connection-based formulation of gravity that does not involve a metric. After a review of basic properties of affine gravity, we compute the tree-level scattering amplitude of scalar particles interacting gravitationally via the connection in a curved spacetime. We find that, while classically equivalent to general relativity, affine gravity differs from metric quantum gravity.

PhysicsHigh Energy Physics - TheorySpacetime010308 nuclear & particles physicsGeneral relativityScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyScattering amplitudeHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesQuantum gravityAffine transformation010306 general physicsMathematical physicsPhysical Review
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Enumerating higher-dimensional operators with on-shell amplitudes

2020

We establish a simple formula for the minimal dimension of operators leading to any helicity amplitude. It eases the systematic enumeration of independent operators from the construction of massless non-factorizable on-shell amplitudes. Little-group constraints can then be solved algorithmically for each helicity configuration to extract a complete set of spinor structures with lowest dimension. Occasionally, further reduction using momentum conservation, on-shell conditions and Schouten identities is required. A systematic procedure to account for the latter is presented. Dressing spinor structures with dot products of momenta finally yields the independent Lorentz structures for each heli…

PhysicsHigh Energy Physics - TheorySpinor010308 nuclear & particles physicsLorentz transformationGravitonFOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesHelicitysymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Dimension (vector space)0103 physical sciencessymbolsEffective field theory010306 general physicsMathematical physicsGauge symmetrySpin-½
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